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Nonlinear second order electromagnetic gyrokinetic theory for a tokamak plasma

Abstract:
Abstract The steep plasma pressure gradient that forms at the edge of the high confinement, H-mode regime of tokamak operation provides free energy to drive electromagnetic micro-instabilities that are widely believed to influence the transport processes in this so-called pedestal region. This high pressure gradient also provides a high current density (bootstrap current), known to influence ballooning mode stability and to be important for driving kink modes in the ideal magneto-hydrodynamic plasma model (so-called peeling-ballooning modes). Furthermore, efficient, steady state future tokamak power plants must operate with a large bootstrap current in the core and especially concerning spherical tokamaks, confinement will be influenced by electromagnetic turbulence. To accommodate these important situations, conventional electromagnetic gyrokinetic theory is extended to incorporate neoclassical effects in the equilibrium drives, allowing B ϑ ∼ B 0 ( B 0 is the confining magnetic field, and B ϑ is its poloidal component). This provides a global gyrokinetic model that self-consistently captures the consequences of large bootstrap current fractions on the equilibrium distribution functions.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1088/1361-6587/acb173

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Role:
Author
ORCID:
0000-0001-6890-3079
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Role:
Author
ORCID:
0000-0003-3333-7470
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Role:
Author
ORCID:
0000-0001-9666-6103
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Role:
Author
ORCID:
0000-0002-0868-211X
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Institution:
University of Oxford
Role:
Author
ORCID:
0000-0001-9621-7404


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Funder identifier:
10.13039/501100000266
Grant:
EP/R034737/1


Publisher:
IOP Publishing
Journal:
Plasma Physics and Controlled Fusion More from this journal
Volume:
65
Issue:
4
Pages:
045010-045010
Publication date:
2023-03-03
DOI:
EISSN:
1361-6587
ISSN:
0741-3335


Language:
English
Keywords:
Pubs id:
1721005
Local pid:
pubs:1721005
Source identifiers:
W4313854929
Deposit date:
2026-06-08
ARK identifier:
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